  The maximum masses for \(L\)  =(65, 70) MeV are consistent with recent observations of massive neutron stars in both cases of \(\Sigma _{Kn}\)  = 300 MeV and 400 MeV, while the masses within the causal limit for \(L\)  = 60 MeV do not reach the range allowable from the observations of most massive neutron stars to date [1]}, [2]} (the green and yellow bands in Fig. REF ). The radius \(R\)  in the stable branches is consistent with observational constraints from gravitational waves of the binary neutron star mergers GW170817 [3]}, [4]}. Also \(R\)  for \(M\simeq 1.3M_\odot \)  lie within the range of the mass and radius deduced from NICER observations of PSR J0030+0451 [5]}, [6]}.
